Ln(3) and Black Hole Entropy
General Relativity and Quantum Cosmology
2017-08-23 v2
Abstract
We review an idea that uses details of the quasinormal mode spectrum of a black hole to obtain the Bekenstein-Hawking entropy of in Loop Quantum Gravity. We further comment on a recent proposal concerning the quasinormal mode spectrum of rotating black holes. We conclude by remarking on a recent proposal to include supersymmetry.
Cite
@article{arxiv.gr-qc/0404055,
title = {Ln(3) and Black Hole Entropy},
author = {Olaf Dreyer},
journal= {arXiv preprint arXiv:gr-qc/0404055},
year = {2017}
}
Comments
Contribution to the Proceedings of the 3rd International Symposium on Quantum Theory and Symmetries, Cincinnati, September 2003, added references to the numerical investigations of Kerr quasinormal modes by Berti et. al